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7. Use the equation above to ll in the following table for the relationship between the radius, temperature, and luminosity of different stars on the

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7. Use the equation above to ll in the following table for the relationship between the radius, temperature, and luminosity of different stars on the Main Sequence. 8. There is also a relationship between mass and luminosity for stars on the Main Sequence: L is proportional to M15 If you use units ofLm and Mm, the formula becomes L = Mas What is the luminosity of a 2 Msun star in units of L5\"? [Do not write units in the box below, just the value] 9. Using the formula above, what is the mass of a star with a luminosity of 3,160 LSun in units of MSun? [Do not write units in the box below, just the value] 10. Return to the HR diagram simulator to answer the following question. Drag your test star around to fill in the blanks about the general trends in the diagram: i) Hot stars are found at the: bottom, left, top, or right ii) Faint stars are found at the: bottom, left, top, or right iii) Luminous (bright) stars are found at the: bottom, left, top, or right iv) Cool staIs are found at the: bottom, left, top, or right

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